Published March 1991
| Version v1
Journal article
Microlensing in the Q0957 + 561 gravitational mirage
Creators
- 1. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)
Description
Analysis of the 10 yr record from monitoring the continuum brightness of Q0957 + 561 A, B shows a systematic increase of the B relative to the A component. The B brightness has leveled off in the last 2 yr at a value 32 percent higher than would be predicted from the ratio of Mg II 2798 A emission line strengths. This is taken to be the signature of microlensing by a star or stars in the lens galaxy. 11 refs
Additional details
Publishing Information
- Journal Title
- Astronomical Journal
- Journal Volume
- 101
- Series
- Astron. J.
- Journal Page Range
- 813-817
- ISSN
- 0004-6256
- CODEN
- ANJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22053417
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCRETION DISKS; BRIGHTNESS; COSMIC GASES; EMISSION SPECTRA; GRAVITATION; GRAVITATIONAL LENSES; INTERSTELLAR SPACE; MASS SPECTRA; QUASARS
- Descriptors DEC
- COSMIC RADIO SOURCES; FLUIDS; GASES; LENSES; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SPACE; SPECTRA